E-viri
Recenzirano
Odprti dostop
-
Aguilar, M; Ambrosi, G; Attig, N; Bagwell, C; Battiston, R; Behlmann, M; Belyaev, N; Bolster, J; Borgia, B; Boschini, M J; Bueno, E F; Burger, W J; Burmeister, S; Castellini, G; Chang, Y H; Chen, H S; Chung, C H; Consolandi, C; Corti, C; Cui, Z; Dadzie, K; Derome, L; Dimiccoli, F; von Doetinchem, P; Egorov, A; Eline, A; Fiandrini, E; Fisher, P; Gámez, C; García-López, R J; Gargiulo, C; Gast, H; Gervasi, M; Giovacchini, F; Grandi, D; Hsieh, T H; Kim, G N; Kounine, A; Laudi, E; Laurenti, G; Lazzizzera, I; Lee, H T; Lee, S C; Li, H L; Li, J Q; Li, S; Liang, J; Light, C; Lu, S Q; Lu, Y S; Luo, J Z; Luo, Xi; Machate, F; Martínez, G; Maurin, D; Mussolin, L; Negrete, J; Nozzoli, F; Ocampo-Peleteiro, J; Orcinha, M; Palermo, M; Pashnin, A; Pensotti, S; Poluianov, S; Qin, X; Rancoita, P G; Rapin, D; Conde, A Reina; Schael, S; von Dratzig, A Schultz; Schwering, G; Seo, E S; Shan, B S; Song, X J; Sonnabend, R; Strigari, L; Tacconi, M; Tang, X W; Tang, Z C; Tian, J; Tomassetti, N; Usoskin, I; Vagelli, V; Vainio, R; Valtonen, E; Vecchi, M; Velasco, M; Wang, C X; Weng, Z L; Wu, H; Yan, Q; Yang, Y; Yi, H; Zhang, C; Zhang, F; Zhang, Z; Zhao, F; Zheng, C; Zhuang, H L; Zichichi, A
Physical review letters, 04/2023, Letnik: 130, Številka: 16Journal Article
We present the precision measurements of 11 years of daily cosmic electron fluxes in the rigidity interval from 1.00 to 41.9 GV based on 2.0×10^{8} electrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The electron fluxes exhibit variations on multiple timescales. Recurrent electron flux variations with periods of 27 days, 13.5 days, and 9 days are observed. We find that the electron fluxes show distinctly different time variations from the proton fluxes. Remarkably, a hysteresis between the electron flux and the proton flux is observed with a significance of greater than 6σ at rigidities below 8.5 GV. Furthermore, significant structures in the electron-proton hysteresis are observed corresponding to sharp structures in both fluxes. This continuous daily electron data provide unique input to the understanding of the charge sign dependence of cosmic rays over an 11-year solar cycle.
Avtor
![loading ... loading ...](themes/default/img/ajax-loading.gif)
Vnos na polico
Trajna povezava
- URL:
Faktor vpliva
Dostop do baze podatkov JCR je dovoljen samo uporabnikom iz Slovenije. Vaš trenutni IP-naslov ni na seznamu dovoljenih za dostop, zato je potrebna avtentikacija z ustreznim računom AAI.
Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Baze podatkov, v katerih je revija indeksirana
Ime baze podatkov | Področje | Leto |
---|
Povezave do osebnih bibliografij avtorjev | Povezave do podatkov o raziskovalcih v sistemu SICRIS |
---|
Vir: Osebne bibliografije
in: SICRIS
To gradivo vam je dostopno v celotnem besedilu. Če kljub temu želite naročiti gradivo, kliknite gumb Nadaljuj.